日本地球惑星科学連合2024年大会

講演情報

[E] ポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM11] Space Weather and Space Climate

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:片岡 龍峰(国立極地研究所)、Aronne Mary(NASA Goddard Space Flight Center)、伴場 由美(国立研究開発法人 情報通信研究機構)、Pulkkinen Antti(NASA Goddard Space Flight Center)

17:15 〜 18:45

[PEM11-P20] Long-Term Trend of bias current obtained from Himawari-8/SEDA-e observation

*長妻 努1坂口 歌織1 (1.国立研究開発法人 情報通信研究機構)

キーワード:高エネルギー粒子、センサー校正、センサー劣化、データ処理

Space environment data acquisition monitor (SEDA) onboard Himawari-8, a Japanese geostationary meteorological satellite, has been operating since Nov. 2014. So Himawari-8 has almost 9 years of observation at Japanese meridian of GEO. SEDA has two sensors. One is high energy electron sensor (SEDA-e) and the other is high energy proton sensor (SEDA-p). SEDA-e measures internal charging currents produced from high energy electrons (from 0.1 to 4.5 MeV) collected by 8 metal plates arranged in a stack. Electron fluxes are estimated from the charging currents in each plates. Since the charging currents are quite small, it needs to be amplified by operational amplifier. This means that bias current is contaminated as an offset of particle flux. Therefore, we need to remove the bias current effect. We use bias current model based on the pre-flight measurements for subtraction. The bias current model is a function of temperature of SEDA-e. This works well for the beginning of Himawari-8/SEDA observation. However, the background flux level tends to be increase as time goes on especially for higher energy channels. This suggests that the bias current tend to be increasing with time goes on. Using more than nine years of SEDA-e and its temperature data, long-term trend of bias current and its relationship with high energy particle environment will be discussed in our presentation.